{
  "annotation_id": "aa3bbf38-c4c8-495f-9bb2-9f0fdc53b749",
  "date_created": "2026-02-17T05:53:12.483000Z",
  "date_modified": "2026-02-17T05:53:12.483000Z",
  "file_hash": "4e153388a0c265c429625db28c3ad73372d3313fba6aed90037e5795d03bcbf8",
  "private": false,
  "record": {
    "abstract": "We develop a unified charge-dependent solar modulation model by solving the three-dimensional Parker transport equation, incorporating a realistic wavy heliospheric current sheet to treat drift effects self-consistently. Using a local interstellar spectrum from GALPROP constrained by Voyager data, we fit the model to time-resolved proton and antiproton fluxes measured by the Alpha Magnetic Spectrometer - 02 (AMS-02) during the solar-quiet period (May 2011 to June 2022). To enable rapid parameter scans, we employ neural-network-based surrogate models to compute propagation and modulation matrices efficiently. The results demonstrate that the model simultaneously describes the observed proton and antiproton fluxes with physically reasonable parameters, providing a unified account of charge-dependent modulation.",
    "arxiv_id": "2601.07649",
    "authors": [
      "Hui-Ming Zhang",
      "Su-Jie Lin",
      "Jie Feng",
      "Jie-Teng Jiang",
      "Li-Li Yang"
    ],
    "categories": [
      "astro-ph.HE",
      "astro-ph.SR",
      "physics.space-ph"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "title": "A Unified Charge-Dependent Modulation Model for AMS-02 Proton and Antiproton Fluxes during Solar Minimum",
    "url": "https://arxiv.org/abs/2601.07649",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "46625e80-b8b4-410d-9f37-4ca21dfeede6",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}